{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:MNBAFUNBPIAQ4L7IWZCLVITVWB","short_pith_number":"pith:MNBAFUNB","schema_version":"1.0","canonical_sha256":"634202d1a17a010e2fe8b644baa275b04ce92156e9773d5238ab10d65997f94b","source":{"kind":"arxiv","id":"1906.06791","version":3},"attestation_state":"computed","paper":{"title":"Excitation of Kerr quasinormal modes in extreme--mass-ratio inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Barry Wardell, Jonathan Thornburg, Maarten van de Meent","submitted_at":"2019-06-16T22:58:12Z","abstract_excerpt":"If a small compact object orbits a black hole, it is known that it can excite the black hole's quasinormal modes (QNMs), leading to high-frequency oscillations (\"wiggles\") in the radiated field at $\\mathcal{J}^+$, and in the radiation-reaction self-force acting on the object after its orbit passes through periapsis. Here we survey the phenomenology of these wiggles across a range of black hole spins and equatorial orbits. In both the scalar-field and gravitational cases we find that wiggles are a generic feature across a wide range of parameter space, and that they are observable in field pert"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1906.06791","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-06-16T22:58:12Z","cross_cats_sorted":[],"title_canon_sha256":"820b11917dba5c135dd728f0f9ba4abe1e9b78e8a503dc5d8cfbcdfd4d0888e8","abstract_canon_sha256":"26c16d4e8c94d2cc6b60c632ff68cebcb76cd811344183b13fc9c27523ce1441"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:51:28.908887Z","signature_b64":"Vj0V9954DfGKF0DjATMCIQ8J2sd/5U9zZpJVy5KQlLX7PnAmVHlPyqI5kNptD96zcPtvuxEWdYp1jFr9MBbUBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"634202d1a17a010e2fe8b644baa275b04ce92156e9773d5238ab10d65997f94b","last_reissued_at":"2026-07-05T00:51:28.908443Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:51:28.908443Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Excitation of Kerr quasinormal modes in extreme--mass-ratio inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Barry Wardell, Jonathan Thornburg, Maarten van de Meent","submitted_at":"2019-06-16T22:58:12Z","abstract_excerpt":"If a small compact object orbits a black hole, it is known that it can excite the black hole's quasinormal modes (QNMs), leading to high-frequency oscillations (\"wiggles\") in the radiated field at $\\mathcal{J}^+$, and in the radiation-reaction self-force acting on the object after its orbit passes through periapsis. Here we survey the phenomenology of these wiggles across a range of black hole spins and equatorial orbits. In both the scalar-field and gravitational cases we find that wiggles are a generic feature across a wide range of parameter space, and that they are observable in field pert"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.06791","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1906.06791/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1906.06791","created_at":"2026-07-05T00:51:28.908501+00:00"},{"alias_kind":"arxiv_version","alias_value":"1906.06791v3","created_at":"2026-07-05T00:51:28.908501+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.06791","created_at":"2026-07-05T00:51:28.908501+00:00"},{"alias_kind":"pith_short_12","alias_value":"MNBAFUNBPIAQ","created_at":"2026-07-05T00:51:28.908501+00:00"},{"alias_kind":"pith_short_16","alias_value":"MNBAFUNBPIAQ4L7I","created_at":"2026-07-05T00:51:28.908501+00:00"},{"alias_kind":"pith_short_8","alias_value":"MNBAFUNB","created_at":"2026-07-05T00:51:28.908501+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26339","citing_title":"Time-domain framework for the Teukolsky equation with a particle source using comoving hyperboloidal coordinates","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2606.17883","citing_title":"Long-Lived Ringing of Near-Extremal Kerr Black Holes Resonantly Driven by Extreme-Mass-Ratio Inspirals","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2605.24704","citing_title":"Shaping black hole resonances I. Black hole ringdown as a spectral filtering process","ref_index":81,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB","json":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB.json","graph_json":"https://pith.science/api/pith-number/MNBAFUNBPIAQ4L7IWZCLVITVWB/graph.json","events_json":"https://pith.science/api/pith-number/MNBAFUNBPIAQ4L7IWZCLVITVWB/events.json","paper":"https://pith.science/paper/MNBAFUNB"},"agent_actions":{"view_html":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB","download_json":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB.json","view_paper":"https://pith.science/paper/MNBAFUNB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1906.06791&json=true","fetch_graph":"https://pith.science/api/pith-number/MNBAFUNBPIAQ4L7IWZCLVITVWB/graph.json","fetch_events":"https://pith.science/api/pith-number/MNBAFUNBPIAQ4L7IWZCLVITVWB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB/action/storage_attestation","attest_author":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB/action/author_attestation","sign_citation":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB/action/citation_signature","submit_replication":"https://pith.science/pith/MNBAFUNBPIAQ4L7IWZCLVITVWB/action/replication_record"}},"created_at":"2026-07-05T00:51:28.908501+00:00","updated_at":"2026-07-05T00:51:28.908501+00:00"}